{"title":"Distribution and Processing of Highly Siderophile Elements in Cratonic Mantle Lithosphere","authors":"S. Aulbach, J. Mungall, D. G. Pearson","doi":"10.2138/RMG.2016.81.5","DOIUrl":null,"url":null,"abstract":"Cratonic lithospheric mantle is composed of predominantly refractory materials that formed at higher mantle potential temperatures ( T P) than recorded in non-cratonic peridotites. It also shows stronger depletion and fractionation of Pd and Pt from Ru, Os and Ir than oceanic, supra-subduction zone or off-cratonic lithospheric mantle, as well as some of the lowest Se and Te contents. The varied response of the highly siderophile elements (HSE: Os, Ir, Ru, Rh, Pt, Pd, Re, Au), and their embedded radioactive decay systems, to changes in oxygen fugacity ( f O2), sulfur fugacity ( f S2) and pressure ( P )—in particular through the impact of these parameters on the stability of the main HSE-bearing sulfide and alloy phases makes them potentially powerful tracers of their melting environment. Therefore, investigation of the HSE systematics of cratonic mantle peridotites, in combination with information from Re–Os isotopes on time-integrated enrichment or depletion, can help us to understand processes leading to mantle differentiation and continental lithosphere formation in the Archean, which are controversial subjects despite decades of research. The longevity of the cratonic lithosphere implies that there was ample opportunity for secondary overprint, obscuring our view of earlier processes. For example, destabilization of platinum-group element (PGE: Os, Ir, Ru, Rh, Pt, Pd) alloy leading to depletions in the compatible PGE, and perhaps Pt, in some cratonic mantle samples may occur in an oxidizing mantle wedge or through interaction with oxidizing small-volume, volatile-rich melts that typically invade cratonic roots. Such melts may eventually deposit S, Pd, Pt and Re and also capture remaining PGE alloys, consistent with the anomalous S-rich character of many kimberlite-borne xenoliths. Their basalt-borne counterparts show additional late effects of subaerial degassing that can deplete volatile elements (S, Re, Os). Basaltic melts can also scavenge PGE alloys at depth, while still sulfide-undersaturated. Such melts, may, …","PeriodicalId":49624,"journal":{"name":"Reviews in Mineralogy & Geochemistry","volume":"60 1","pages":"239-304"},"PeriodicalIF":0.0000,"publicationDate":"2016-01-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"87","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Reviews in Mineralogy & Geochemistry","FirstCategoryId":"89","ListUrlMain":"https://doi.org/10.2138/RMG.2016.81.5","RegionNum":1,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q1","JCRName":"Earth and Planetary Sciences","Score":null,"Total":0}
引用次数: 87
Abstract
Cratonic lithospheric mantle is composed of predominantly refractory materials that formed at higher mantle potential temperatures ( T P) than recorded in non-cratonic peridotites. It also shows stronger depletion and fractionation of Pd and Pt from Ru, Os and Ir than oceanic, supra-subduction zone or off-cratonic lithospheric mantle, as well as some of the lowest Se and Te contents. The varied response of the highly siderophile elements (HSE: Os, Ir, Ru, Rh, Pt, Pd, Re, Au), and their embedded radioactive decay systems, to changes in oxygen fugacity ( f O2), sulfur fugacity ( f S2) and pressure ( P )—in particular through the impact of these parameters on the stability of the main HSE-bearing sulfide and alloy phases makes them potentially powerful tracers of their melting environment. Therefore, investigation of the HSE systematics of cratonic mantle peridotites, in combination with information from Re–Os isotopes on time-integrated enrichment or depletion, can help us to understand processes leading to mantle differentiation and continental lithosphere formation in the Archean, which are controversial subjects despite decades of research. The longevity of the cratonic lithosphere implies that there was ample opportunity for secondary overprint, obscuring our view of earlier processes. For example, destabilization of platinum-group element (PGE: Os, Ir, Ru, Rh, Pt, Pd) alloy leading to depletions in the compatible PGE, and perhaps Pt, in some cratonic mantle samples may occur in an oxidizing mantle wedge or through interaction with oxidizing small-volume, volatile-rich melts that typically invade cratonic roots. Such melts may eventually deposit S, Pd, Pt and Re and also capture remaining PGE alloys, consistent with the anomalous S-rich character of many kimberlite-borne xenoliths. Their basalt-borne counterparts show additional late effects of subaerial degassing that can deplete volatile elements (S, Re, Os). Basaltic melts can also scavenge PGE alloys at depth, while still sulfide-undersaturated. Such melts, may, …
克拉通岩石圈地幔主要由耐火物质组成,形成于比非克拉通橄榄岩记录的更高的地幔位温(T P)。Pd和Pt在Ru、Os和Ir中的损耗和分馏作用强于大洋、超俯冲带和克拉通外岩石圈地幔,Se和Te含量也处于最低水平。高亲铁元素(HSE: Os, Ir, Ru, Rh, Pt, Pd, Re, Au)及其嵌入的放射性衰变系统对氧逸度(fo2),硫逸度(fs2)和压力(P)变化的不同响应,特别是通过这些参数对主要含硒硫化物和合金相稳定性的影响,使它们成为其熔化环境的潜在强大示踪剂。因此,研究克拉通地幔橄榄岩的HSE系统,结合Re-Os同位素的时间整合富集或衰竭信息,可以帮助我们了解太古宙地幔分异和大陆岩石圈形成的过程,这一问题在几十年的研究中一直存在争议。克拉通岩石圈的长寿意味着有足够的机会进行二次套印,模糊了我们对早期过程的看法。例如,在一些克拉通地幔样品中,铂族元素(PGE: Os, Ir, Ru, Rh, Pt, Pd)合金的失稳导致相容的PGE和Pt的耗尽,可能发生在氧化地幔楔中,或者通过与氧化小体积、富含挥发物的熔体相互作用,这些熔体通常侵入克拉通根部。这些熔体可能最终沉积S、Pd、Pt和Re,并捕获剩余的PGE合金,这与许多金伯利岩捕虏体的异常富S特征一致。玄武岩上的对应物显示出地面脱气的额外后期效应,可以耗尽挥发性元素(S, Re, Os)。玄武岩熔体也可以在硫化物不饱和的情况下清除PGE合金。这样的融化,可能……
期刊介绍:
RiMG is a series of multi-authored, soft-bound volumes containing concise reviews of the literature and advances in theoretical and/or applied mineralogy, crystallography, petrology, and geochemistry. The content of each volume consists of fully developed text which can be used for self-study, research, or as a text-book for graduate-level courses. RiMG volumes are typically produced in conjunction with a short course but can also be published without a short course. The series is jointly published by the Mineralogical Society of America (MSA) and the Geochemical Society.